Space weathering from Mercury to the asteroid belt

By B. Hapke. 2001

830 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/fb136a10f26db0ce595d0f31cee40d86b48ecdbe

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Citations in the corpus

Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes (2004, background): “) Current m els suggest that space weathering processes indeed m effective very rapidly, perhaps in as little as 50,000 ye (Hapke, 2001) , a time that appears very short compared collisional timescales.”
Processes that Promote and Deplete the Exosphere of Mercury (2007, background): “For the surface deeper layers are believed to be less contaminated by space weathering (Hapke 2001), the detection of the vaporized soil due to such impulsive events could be the only way to remote sense the real Hermean endogenous material.”
Mercury’s Weather-Beaten Surface: Understanding Mercury in the Context of Lunar and Asteroidal Space Weathering Studies (2014, methodology): “If FeO is present, then hydrogen implantation will reduce the FeO to Fe0, forming single-domain, nanometer-scale metallic iron particles within the upper layers of the regolith grains (Hapke 2001).”
Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification (2012, methodology): “If we consider that an amount of ∼ 0.02% of SMFe is required to explain the red slopes of some S-complex asteroids (e.g., Hapke, 2001; Rivkin et al., 2004), this means that the spectral slope for the highest phase angle (g = 120o) would be equivalent to ∼ 30% of that SMFe.”
SPACE WEATHERING OF ASTEROID SURFACES (2004, methodology): “Following Hapke (2001), they model four processes or factors: (a) amount of submicroscopic vapor-deposited iron, (b) a neutral, opaque component (perhaps admixed carbonaceous material or darkening by shock), (c) particle size, and (d) composition (I’ve noted above that olivine is especially…”
Evidence for asteroid space weathering from the Sloan Digital Sky Survey (2005, background): “Studies of soils and rocks collected by the Apollo tronauts provide evidence for processes that alter op properties of the lunar surface (e.g.,Hapke (2001)and references therein).”
Asteroid Space Weathering and Regolith Evolution (2002, methodology): “The model is described in detail in Hapke (2001) and will only be summarized here.”
An experimental approach to understanding the optical effects of space weathering (2007, background): “…repeatedly suggested that the spectral differences between Stype asteroids and ordinary chondrites can be accounted for by very small amounts of lunar-like space weathering products (i.e. npFe0-bearing rims) (e.g. Binzel et al., 1996; Pieters et al., 2000; Hapke, 2001; Noble et al., 2004, 2006).”
Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids (2017, background): “The importance of npFe0 in these 18 AC CE PT ED M AN US CR IP T modifications has been underlined by many authors [Hapke, 2001; Noble et al., 2007] and their presence confirmed on S-type NEA Itokawa (Hayabusa/JAXA mission) [Hiroi et al., 2006; Yoshikawa et al., 2007] as a result of solar wind…”